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Lyman-Werner escape fractions from the first galaxies

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Direct collapse black holes forming in pristine, atomically cooling haloes at z ≈ 10-20 may act as the seeds of supermassive black holes (BHs) at high redshifts. In order to create a massive BH seed, the host halo needs to be prevented from forming stars. H2 therefore needs to be irradiated by a lar...

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Main Authors: Schauer, Anna T. P. (Author) , Glover, Simon (Author) , Klessen, Ralf S. (Author)
Format: Article (Journal)
Language:English
Published: 22 February 2017
In: Monthly notices of the Royal Astronomical Society
Year: 2017, Volume: 467, Issue: 2, Pages: 2288-2300
ISSN:1365-2966
DOI:10.1093/mnras/stx264
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stx264
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Author Notes:Anna T.P. Schauer, Bhaskar Agarwal, Simon C.O. Glover, Ralf S. Klessen, Muhammad A. Latif, Lluís Mas-Ribas, Claes-Erik Rydberg, Daniel J. Whalen and Erik Zackrisson
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Lyman-Werner escape fractions from the first galaxies by Schauer, Anna T. P. (Author) , Glover, Simon (Author) , Klessen, Ralf S. (Author) ,


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